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How likely is it that when stars are orbiting the centre of a galaxy that two stars will meet and be locked together and orbit each other or collide?
The likelihood of stars colliding or becoming gravitationally bound while orbiting the center of a galaxy is extremely low due to the vast distances between them. Even during the anticipated collision of the Milky Way with the Andromeda galaxy, such events will remain rare. Collisions typically occur between stars that have been in close proximity for extended periods, often resulting from degrading orbits or mass loss during stellar evolution. Gamma-ray bursts are associated with the merger of neutron stars or interactions with black holes, indicating that while rare on human timescales, such events are more common over the lifespan of stars.
PREREQUISITESAstronomers, astrophysics students, and anyone interested in the dynamics of star interactions and the evolution of galaxies.